The microwave pulsations in solar flares - Magnetohydrodynamic and plasma models

Details The microwave pulsations in solar flares - Magnetohydrodynamic and plasma models The microwave pulsations in solar flares - Magnetohydrodynamic and plasma models

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985pazh...11..463z&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 11, June 1985, p. 463-468) Soviet Astronomy Letters (ISSN 0360-0327), vol. 11, May-June

Astronomy and Astrophysics

Astronomy

2

Magnetohydrodynamic Waves, Microwave Spectra, Plasma Waves, Pulsed Radiation, Solar Flares, Stellar Models, Magnetohydrodynamic Stability, Plasma Diagnostics

Scientific paper

The approximately 1-sec microwave pulsations observed in solar flares are attributable to MHD oscillations of the flare loop resulting from the sudden energy release. The millisecond pulsations, on the other hand, result from a nonlinear oscillation regime of loss-cone instability for the plasma waves in the flare loop. Both types of microwave pulsation are useful for flare-plasma diagnostics.

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